WO2019071917A1 - Satellite tracking method - Google Patents

Satellite tracking method Download PDF

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WO2019071917A1
WO2019071917A1 PCT/CN2018/080033 CN2018080033W WO2019071917A1 WO 2019071917 A1 WO2019071917 A1 WO 2019071917A1 CN 2018080033 W CN2018080033 W CN 2018080033W WO 2019071917 A1 WO2019071917 A1 WO 2019071917A1
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antenna
function
angle
satellite
rssi
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PCT/CN2018/080033
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French (fr)
Chinese (zh)
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杨飞
袁世钊
刘冰
吴晓文
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深圳市华讯方舟空间信息产业科技有限公司
华讯方舟科技有限公司
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Publication of WO2019071917A1 publication Critical patent/WO2019071917A1/en

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    • GPHYSICS
    • G01MEASURING; TESTING
    • G01SRADIO DIRECTION-FINDING; RADIO NAVIGATION; DETERMINING DISTANCE OR VELOCITY BY USE OF RADIO WAVES; LOCATING OR PRESENCE-DETECTING BY USE OF THE REFLECTION OR RERADIATION OF RADIO WAVES; ANALOGOUS ARRANGEMENTS USING OTHER WAVES
    • G01S19/00Satellite radio beacon positioning systems; Determining position, velocity or attitude using signals transmitted by such systems
    • G01S19/01Satellite radio beacon positioning systems transmitting time-stamped messages, e.g. GPS [Global Positioning System], GLONASS [Global Orbiting Navigation Satellite System] or GALILEO
    • G01S19/13Receivers
    • G01S19/24Acquisition or tracking or demodulation of signals transmitted by the system

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  • the present invention relates to the field of electromagnetic beam tracking, and in particular to a satellite tracking method.
  • High-precision acquisition and tracking of satellite signals has always been a core indicator of satellite antennas.
  • Most of the current methods of automatic tracking satellites involve hardware analysis of satellite signal power level values rssi for beam signal indication.
  • the current satellite tracking algorithm is a simple processing of the satellite beam signal value. By stepping the vicinity of the incoming beam and searching for the maximum point of the signal, as a star-based basis, the signal processing method is very simple. There is a large delay, the error is also large, and the precision needs to be improved.
  • the partial scanning method is only based on the way of finding the maximum signal position.
  • This processing mechanism has no problem for single-sided reception, but there is also a shortage for antenna transmission, because the antenna transmission and reception main lobe cannot be guaranteed during antenna design and installation.
  • the axes are completely coincident, and the inconsistent transmission and reception frequency points also cause the directivity coefficient function of the transmitting and receiving beams to be inconsistent. If the received signal strength is simply analyzed, the transmission beam pattern characteristics will be affected, and the transmission gain performance and the cross polarization isolation will be affected.
  • a satellite tracking method for achieving fast alignment of satellites including:
  • the compensation angle is dynamically acquired during the alignment process, and the antenna scan tracking alignment satellite is continuously adjusted according to the compensation angle.
  • the step of acquiring a directivity coefficient function of the antenna includes:
  • a fitting function model fitting corresponding to the antenna is selected according to the far field direction coefficient data to generate a directivity coefficient function.
  • the step of collecting direction coefficient data of different frequency bands of the antenna includes:
  • the fit function model is:
  • J 1 (x) is a first-order Bessel function
  • u [Az El]
  • Az is the azimuth difference of the antenna obtained by the actual measurement of the antenna microwave darkroom
  • El is the difference of the pitch angle of the antenna obtained by the actual measurement of the antenna microwave darkroom
  • h is a constant, which is automatically generated by function fitting
  • the fit function model is:
  • Az is the azimuth difference of the antenna obtained by the actual measurement of the antenna microwave darkroom
  • El is the difference of the pitch angle of the antenna obtained by the actual measurement of the antenna microwave darkroom
  • h is a constant, which is automatically generated by function fitting
  • the obtaining a Jacobian matrix of the directivity coefficient function is used for determining an angle compensation direction of the antenna, comprising:
  • D( ⁇ n ) is another representation of D(Az, El).
  • the obtaining, by scanning, a matrix of deviation angles of the antenna relative to a satellite, the deviation angle matrix being used to provide a function model for obtaining a compensation angle comprising:
  • the scan range function Gk(rssi) is based on the PI filter principle:
  • Is a constant
  • rssi n and rssi k respectively represent the collected values of the nth and kth rssi
  • Kp is a proportional amplification factor
  • Ki is an integral amplification factor
  • the spiral progressive scan is performed by automatically changing the size of the scan range value of the scan range function.
  • the acquiring the compensation angle according to the directivity coefficient function, the deviation angle matrix, and the Jacobian matrix, the compensation angle is used to guide the antenna to move at a next moment. Steps, including:
  • ⁇ n-1 is the deviation angle matrix value at time n-1
  • rssi n is the collected value of the nth rssi
  • It is a Jacobian matrix
  • D(Az, El) is the actual directivity coefficient function
  • ⁇ t is the algorithm iteration period
  • is the adjustment step size, and the values of different types of antennas ⁇ are different.
  • the step of dynamically acquiring the compensation angle during the alignment process and continuously adjusting the antenna scan tracking alignment satellite according to the compensation angle includes:
  • the spiral progressive scan is performed by automatically changing the size of the scan range value of the scan range function
  • the scan range function Gk(rssi) is based on the principle of the PI filter:
  • Gk n represents the output value of the nth Gk(rssi) function, ie the scan range value
  • rssi max is a theoretically calculated value, which is a constant
  • rssi n and rssi k represent the nth and kth rssi respectively Collected value
  • Kp is a proportional amplification factor
  • Ki is an integral amplification factor
  • whether the satellite is aligned is determined by a signal quality indicator of the satellite receiver.
  • the above satellite tracking method quickly converges the satellite tracking error by collecting less or lower frequency beam signal data, and continuously tracks the alignment satellite by continuously obtaining the compensation angle, thereby improving the accuracy of satellite alignment and the accuracy of beam tracking, and reducing Delay and error. At the same time, it can be well adapted to the needs of various satellite beam tracking. Make full use of existing hardware condition resources without adding additional equipment, which reduces the dependence on the accuracy of servo drive system and attitude inertial navigation system.
  • 1 is a flow chart of a satellite tracking method in an example
  • FIG. 2 is a flow chart of obtaining a directivity coefficient function of an antenna in an embodiment.
  • the satellite tracking method is used to implement fast tracking alignment of satellites, and includes the following steps S100-S500.
  • step S100 a directivity coefficient function of the antenna is obtained.
  • the directivity coefficient of the antenna is used to indicate the degree of concentrated radiation of the antenna, and is specifically defined as the ratio of the radiated power density of the antenna in the maximum radiation direction to the radiated power density of the uniform radiation in the direction in the case where the total radiated power is the same.
  • the directivity coefficient of the antenna is actually the directivity coefficient function of the antenna. Firstly, according to different antenna types, the theoretical calculation is carried out, and the direction pattern data of the antenna obtained by the antenna microwave darkroom test is combined, and the obtained direction pattern data is synthesized into a pattern by the averaging method. A regression fit is applied to the pattern to generate a directivity coefficient function.
  • a process for generating a directivity coefficient function of an antenna includes:
  • Step S110 collecting direction coefficient data of different frequency bands of the antenna.
  • the directional coefficient data of the antenna receiving frequency band and the transmitting frequency band are collected.
  • the receiving frequency band is 18.7 to 19.2, and the transmitting frequency band is 29.5 to 30.0.
  • 10 frequency points are extracted from the medium interval in the receive band. Extract 10 frequency points from the medium interval in the transmit band.
  • the 20 sets of pattern data corresponding to the 20 frequency points are respectively collected in the antenna microwave darkroom.
  • this collection method is not limited, and data acquisition can be performed on different satellite antennas according to actual operations and needs.
  • Step S120 converting direction coefficient data of the different frequency bands to generate far-field direction coefficient data.
  • the collected direction coefficient data of the antenna receiving frequency band is converted to generate far-field direction coefficient data; and the direction coefficient data of the collected antenna transmitting frequency band is converted to generate far-field direction coefficient data.
  • Step S130 selecting a fitting function model corresponding to the antenna to generate a directivity coefficient function according to the far field direction coefficient data.
  • the fitting function model is:
  • J 1 (x) is a first-order Bessel function
  • Bezier function J ⁇ (x) is a general term for a class of special functions in mathematics.
  • the Bessel function is the solution of the Bessel equation.
  • is called the order of its corresponding Bessel function.
  • the most common case in practical applications is that ⁇ is an integer n and the corresponding solution is called an n-order Bessel function.
  • J 1 (x) is the solution of the corresponding Bessel equation when n is 1.
  • Bessel function u is a one-dimensional array containing two angle values, one H-direction deviation angle, and one V-direction deviation angle.
  • Az is the azimuth difference value of the antenna obtained by the actual measurement of the antenna microwave darkroom
  • El is the difference of the pitch angle of the antenna obtained by the actual measurement of the antenna microwave darkroom
  • h is a constant, which is automatically generated by function fitting
  • the fit function model is:
  • J 1 (x) is a first-order Bessel function
  • x u
  • u [Az El]
  • Az is the azimuth difference of the antenna obtained by the actual measurement of the antenna microwave darkroom
  • El is the difference of the pitch angle of the antenna obtained by the actual measurement of the antenna microwave darkroom
  • h is a constant, which is automatically generated by function fitting
  • Step S200 Acquire a Jacobian matrix of the directivity coefficient function, and the Jacobian matrix is used to determine an angle compensation direction of the antenna.
  • the obtained directional coefficient function is subjected to partial differential derivation to obtain a Jacobian matrix
  • the Jacobian matrix can be obtained by the following formula:
  • D(Az, El) is the actual direction coefficient function generated by the simulation
  • Step S300 obtaining, by scanning, a matrix of deviation angles of the antenna with respect to a satellite, wherein the deviation angle matrix is used to provide a function model for acquiring a compensation angle.
  • a matrix of deviation angles of the antenna relative to a satellite is obtained by scanning, the deviation angle matrix is used to provide a function model for acquiring a compensation angle; and the actual azimuth difference value Az of the antenna is obtained by scanning measurement , pitch angle difference E1; Then ⁇ satisfies:
  • Gk(rssi) is the sweep range function of the antenna, the size is determined by the antenna beam signal value rssi value; K Az is the scan scale factor of the azimuth deviation angle, K El is the scan scale factor of the pitch deviation angle, and the scan scale factor is It is determined by the type of antenna.
  • the scan range function Gk(rssi) is based on the PI filter principle:
  • rssi n and rssi k respectively represent the collected values of the nth and kth rssi; according to the principle of the PI filter, Kp is a proportional amplification factor; Ki is an integral amplification factor;
  • the spiral progressive scan is performed by automatically changing the size of the scan range value Gk n of the scan range function.
  • Step S400 Acquire the compensation angle according to the directivity coefficient function, the deviation angle matrix, and the Jacobian matrix, where the compensation angle is used to guide the antenna to move at a next moment.
  • the compensation angle is used to guide the antenna to move at a next moment.
  • the obtained directivity coefficient function, deviation angle matrix, and Jacobian matrix are substituted into the formula to obtain the compensation angle. Further, the following formula can be used to obtain the compensation angle:
  • ⁇ n-1 is the deviation angle matrix value at time n-1
  • rssi n is the collected value of the nth rssi
  • It is a Jacobian matrix
  • D(Az, El) is the actual directivity coefficient function
  • ⁇ t is the algorithm iteration period
  • is the adjustment step size, and the values of different types of antennas ⁇ are different.
  • the current time is the time n-1, where the value of ⁇ n-1 is actually measured, and the value of ⁇ n obtained from the value of ⁇ n-1 is used to guide the angle at which the antenna is to be moved at the next moment. .
  • Step S500 dynamically acquiring the compensation angle during the alignment process, and continuously adjusting the antenna scan tracking alignment satellite according to the compensation angle.
  • the compensation angle is dynamically acquired during the alignment process, and the antenna scan tracking alignment satellite is continuously adjusted according to the compensation angle.
  • the spiral scanning method is adopted for the scanning method of the satellite, and the spiral progressive scanning is performed by automatically changing the scanning range value of the scanning range function.
  • the scan range function Gk(rssi) is based on the principle of the PI filter:
  • Gk n represents the output value of the nth Gk(rssi) function, ie the scan range value
  • rssi max is a theoretically calculated value, which is a constant
  • rssi n and rssi k represent the nth and kth rssi respectively Collected value
  • Kp is a proportional amplification factor
  • Ki is an integral amplification factor
  • whether the satellite is aligned is determined by a signal quality indicator of the satellite receiver. Specifically, when the received signal strength indication reaches 70% to 80%, it indicates that the antenna has been aligned with the general orientation of the satellite. When the signal quality is about 40%, it indicates that the satellite is aligned, and the signal may be eb/ The n0 value is used to determine if the satellite is aligned.
  • the first large-scale signal scanning is performed to make the antenna substantially face the satellite beam, and then the directional coefficient function is obtained through the darkroom simulation, and then the directional coefficient function is used to solve the partial differential function to determine the angle compensation direction and the compensation angle.
  • the spiral progressive scan is realized by changing the scan range value, so that the antenna can realize fast tracking and alignment to the satellite, and the accuracy of the antenna beam pointing is improved; and the compensation angle of the antenna can be automatically adjusted according to different dynamic characteristics to adapt the satellite; Making full use of existing hardware resources, without adding additional equipment, reduces the dependence of tracking accuracy on servo systems and attitude inertial navigation systems.

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  • Radar, Positioning & Navigation (AREA)
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Abstract

A satellite tracking method, which is used for the fast tracking and alignment of satellites, comprising: acquiring a directional coefficient function of an antenna (S100); acquiring a Jacobian matrix of the directional coefficient function, the Jacobian matrix being used for determining a direction of angle compensation for the antenna (S200); acquiring a deviation angle matrix of the antenna relative to a satellite by means of scanning, the deviation angle matrix being used for providing a function model in order to acquire a compensation angle (S300); acquiring the compensation angle according to the directional coefficient function, the deviation angle matrix and the Jacobian matrix, the compensation angle being used for guiding the antenna to move at a next moment; dynamically acquiring the compensation angle and continuously adjusting the antenna according to the compensation angle during a process of alignment so as to scan, track and align the satellite (S500). A satellite tracking error is rapidly converged by means of acquiring less or lower-frequency beam signal data, thus implementing high-precision satellite alignment.

Description

卫星跟踪方法Satellite tracking method 技术领域Technical field
本发明涉及电磁波束跟踪领域,特别是涉及一种卫星跟踪方法。The present invention relates to the field of electromagnetic beam tracking, and in particular to a satellite tracking method.
背景技术Background technique
高精度的捕获跟踪卫星信号一直是卫星天线一项核心指标,当前大部分自动跟踪卫星方法都是会涉硬件解析卫星信号的功率电平值rssi来做波束信号指示。当前卫星跟踪算法都是对卫星波束信号值的简单处理,通过对来波束附近做步进扫描,搜寻信号最大点,作为对星依据,信号处理方式很简单。存在较大的时延,误差也大,精度也待提高。High-precision acquisition and tracking of satellite signals has always been a core indicator of satellite antennas. Most of the current methods of automatic tracking satellites involve hardware analysis of satellite signal power level values rssi for beam signal indication. The current satellite tracking algorithm is a simple processing of the satellite beam signal value. By stepping the vicinity of the incoming beam and searching for the maximum point of the signal, as a star-based basis, the signal processing method is very simple. There is a large delay, the error is also large, and the precision needs to be improved.
而且,部分扫描方式仅依据寻找接收最大信号位置方式,这种处理机制对于单边接收没有问题,但是对于天线发射也会存在不足,因为天线设计时和安装过程中,无法保证天线收发波主瓣轴线完全重合,同时收发频点不一致也导致收发波束的方向性系数函数肯定不一致,若简单分析接收的信号强度,不考虑发射波束方向图特性,会影响发射增益性能,发射交叉极化隔离度。Moreover, the partial scanning method is only based on the way of finding the maximum signal position. This processing mechanism has no problem for single-sided reception, but there is also a shortage for antenna transmission, because the antenna transmission and reception main lobe cannot be guaranteed during antenna design and installation. The axes are completely coincident, and the inconsistent transmission and reception frequency points also cause the directivity coefficient function of the transmitting and receiving beams to be inconsistent. If the received signal strength is simply analyzed, the transmission beam pattern characteristics will be affected, and the transmission gain performance and the cross polarization isolation will be affected.
发明内容Summary of the invention
基于此,有必要针对精度低、误差大、有时延等问题,提供一种卫星跟踪方法。Based on this, it is necessary to provide a satellite tracking method for problems such as low precision, large error, and delay.
一种卫星跟踪方法,用于实现卫星的快速对准,包括:A satellite tracking method for achieving fast alignment of satellites, including:
获取天线的方向性系数函数;Obtaining a directivity coefficient function of the antenna;
获取所述方向性系数函数的雅可比矩阵,所述雅可比矩阵用于确定所述天线的角度补偿方向;Obtaining a Jacobian matrix of the directivity coefficient function, wherein the Jacobian matrix is used to determine an angle compensation direction of the antenna;
通过扫描获取所述天线相对于卫星的偏差角矩阵,所述偏差角矩阵用于为获取补偿角度提供函数模型;Obtaining, by scanning, a matrix of deviation angles of the antenna relative to a satellite, the deviation angle matrix being used to provide a function model for acquiring a compensation angle;
根据所述方向性系数函数、所述偏差角矩阵、所述雅可比矩阵获取所述补 偿角度,所述补偿角度用于指导所述天线在下一时刻进行移动;Obtaining the compensation angle according to the directivity coefficient function, the deviation angle matrix, and the Jacobian matrix, wherein the compensation angle is used to guide the antenna to move at a next moment;
在对准过程中动态获取所述补偿角度,并根据所述补偿角度不断调整所述天线扫描跟踪对准卫星。The compensation angle is dynamically acquired during the alignment process, and the antenna scan tracking alignment satellite is continuously adjusted according to the compensation angle.
在其中一个实施例中,所述获取天线的方向性系数函数的步骤,包括:In one embodiment, the step of acquiring a directivity coefficient function of the antenna includes:
采集天线不同频段的方向系数数据;Collecting direction coefficient data of different frequency bands of the antenna;
将所述不同频段的方向系数数据转换生成远场方向系数数据;Converting the direction coefficient data of the different frequency bands to generate far-field direction coefficient data;
根据所述远场方向系数数据选择与所述天线对应的拟合函数模型拟合生成方向性系数函数。A fitting function model fitting corresponding to the antenna is selected according to the far field direction coefficient data to generate a directivity coefficient function.
在其中一个实施例中,所述采集天线不同频段的方向系数数据的步骤,包括:In one embodiment, the step of collecting direction coefficient data of different frequency bands of the antenna includes:
采集天线接收频段、发射频段的方向系数数据。Collect the direction coefficient data of the antenna receiving band and the transmitting band.
在其中一个实施例中,对于平面阵列天线,所述拟合函数模型为:In one of the embodiments, for a planar array antenna, the fit function model is:
Figure PCTCN2018080033-appb-000001
Figure PCTCN2018080033-appb-000001
其中J 1(x)为一阶贝塞尔函数,
Figure PCTCN2018080033-appb-000002
u=[Az El],
Where J 1 (x) is a first-order Bessel function,
Figure PCTCN2018080033-appb-000002
u=[Az El],
Az为通过天线微波暗室实际测量获取的天线的方位角差值;El为通过天线微波暗室实际测量获取的天线的俯仰角差值;h为常数,通过函数拟合时自动生成;Az is the azimuth difference of the antenna obtained by the actual measurement of the antenna microwave darkroom; El is the difference of the pitch angle of the antenna obtained by the actual measurement of the antenna microwave darkroom; h is a constant, which is automatically generated by function fitting;
将所述方位角差值Az和俯仰角差值El代入所述函数模型后得到方向性系数函数D(Az,El);Substituting the azimuth difference value Az and the pitch angle difference value El into the function model to obtain a directivity coefficient function D(Az, El);
对于反射面天线,所述拟合函数模型为:For a reflector antenna, the fit function model is:
Figure PCTCN2018080033-appb-000003
Figure PCTCN2018080033-appb-000003
其中J 1(x)为一阶贝塞尔函数,x=u;u=[Az El]; Where J 1 (x) is a first-order Bessel function, x=u; u=[Az El];
Az为通过天线微波暗室实际测量获取的天线的方位角差值;El为通过天线微波暗室实际测量获取的天线的俯仰角差值;h为常数,通过函数拟合时自动生成;Az is the azimuth difference of the antenna obtained by the actual measurement of the antenna microwave darkroom; El is the difference of the pitch angle of the antenna obtained by the actual measurement of the antenna microwave darkroom; h is a constant, which is automatically generated by function fitting;
将所述天线的方位角差值Az和俯仰角差值El代入所述函数模型后得到方向性系数函数D(Az,El)。Substituting the azimuth difference value Az and the pitch angle difference value E of the antenna into the function model yields a directivity coefficient function D(Az, El).
在其中一个实施例中,所述获取所述方向性系数函数的雅可比矩阵,所述雅可比矩阵用于确定所述天线的角度补偿方向的步骤,包括:In one embodiment, the obtaining a Jacobian matrix of the directivity coefficient function, the Jacobian matrix is used for determining an angle compensation direction of the antenna, comprising:
所述
Figure PCTCN2018080033-appb-000004
Said
Figure PCTCN2018080033-appb-000004
其中,
Figure PCTCN2018080033-appb-000005
among them,
Figure PCTCN2018080033-appb-000005
其中,D(Δθ n)为D(Az,El)的另一种表示形式。 Where D(Δθ n ) is another representation of D(Az, El).
在其中一个实施例中,所述通过扫描获取所述天线相对于卫星的偏差角矩阵,所述偏差角矩阵用于为获取补偿角度提供函数模型的步骤,包括:In one embodiment, the obtaining, by scanning, a matrix of deviation angles of the antenna relative to a satellite, the deviation angle matrix being used to provide a function model for obtaining a compensation angle, comprising:
通过扫描测量获取天线实际的方位角差值Az、俯仰角差值El,设所述
Figure PCTCN2018080033-appb-000006
Figure PCTCN2018080033-appb-000007
则Δθ满足:
Obtaining the actual azimuth difference Az and the elevation angle difference El of the antenna by scanning measurement,
Figure PCTCN2018080033-appb-000006
Figure PCTCN2018080033-appb-000007
Then Δθ satisfies:
Figure PCTCN2018080033-appb-000008
Figure PCTCN2018080033-appb-000008
Figure PCTCN2018080033-appb-000009
Figure PCTCN2018080033-appb-000009
其中,
Figure PCTCN2018080033-appb-000010
为偏差角角速度矩阵,
Figure PCTCN2018080033-appb-000011
为Δθ对时间的求导;H=ωK,H为常数系数;其中Gk(rssi)为扫描范围函数,大小由天线波束信号值rssi值决定;K Az、K El为扫描比例系数。
among them,
Figure PCTCN2018080033-appb-000010
For the angular angular velocity matrix,
Figure PCTCN2018080033-appb-000011
It is the derivative of Δθ versus time; H=ωK, H is a constant coefficient; where Gk(rssi) is a function of the scan range, and the size is determined by the value of the antenna beam signal value rssi; K Az and K El are the scan scale coefficients.
在其中一个实施例中,所述扫描范围函数Gk(rssi)依据PI滤波器原理:In one of the embodiments, the scan range function Gk(rssi) is based on the PI filter principle:
Figure PCTCN2018080033-appb-000012
为一个常数;rssi n、rssi k分别表示第n次、第k次rssi的采集值;Kp为比例放大系数;Ki为积分放大系数;
Figure PCTCN2018080033-appb-000012
Is a constant; rssi n and rssi k respectively represent the collected values of the nth and kth rssi; Kp is a proportional amplification factor; Ki is an integral amplification factor;
其中,通过自动变更扫描范围函数的扫描范围值的大小来进行螺旋渐进扫描。Among them, the spiral progressive scan is performed by automatically changing the size of the scan range value of the scan range function.
在其中一个实施例中,所述根据所述方向性系数函数、所述偏差角矩阵、所述雅可比矩阵获取所述补偿角度,所述补偿角度用于指导所述天线在下一时刻进行移动的步骤,包括:In one embodiment, the acquiring the compensation angle according to the directivity coefficient function, the deviation angle matrix, and the Jacobian matrix, the compensation angle is used to guide the antenna to move at a next moment. Steps, including:
所述补偿角度
Figure PCTCN2018080033-appb-000013
The compensation angle
Figure PCTCN2018080033-appb-000013
其中,among them,
Figure PCTCN2018080033-appb-000014
Figure PCTCN2018080033-appb-000014
Figure PCTCN2018080033-appb-000015
为计算的中间变量;Δθ n-1为n-1时刻的偏差角矩阵值;rssi n为第n次rssi的采集值;
Figure PCTCN2018080033-appb-000016
为雅可比矩阵;D(Az,El)为实际方向性系数函数;Δt为算法迭代周期;β为调节步长,对于不同类型的天线β的取值不同。
Figure PCTCN2018080033-appb-000015
For the calculated intermediate variable; Δθ n-1 is the deviation angle matrix value at time n-1; rssi n is the collected value of the nth rssi;
Figure PCTCN2018080033-appb-000016
It is a Jacobian matrix; D(Az, El) is the actual directivity coefficient function; Δt is the algorithm iteration period; β is the adjustment step size, and the values of different types of antennas β are different.
在其中一个实施例中,所述在对准过程中动态获取所述补偿角度,并根据所述补偿角度不断调整所述天线扫描跟踪对准卫星的步骤,包括:In one embodiment, the step of dynamically acquiring the compensation angle during the alignment process and continuously adjusting the antenna scan tracking alignment satellite according to the compensation angle includes:
根据所述补偿角度不断调整所述天线的方位角差值Az和俯仰角差值El螺旋渐进扫描跟踪对准卫星;And continuously adjusting the azimuth difference value Az and the pitch angle difference value of the antenna according to the compensation angle; the spiral progressive scan tracking alignment satellite;
其中,通过自动变更扫描范围函数的扫描范围值的大小来进行螺旋渐进扫描,Wherein, the spiral progressive scan is performed by automatically changing the size of the scan range value of the scan range function,
所述扫描范围函数Gk(rssi)依据PI滤波器原理:The scan range function Gk(rssi) is based on the principle of the PI filter:
Figure PCTCN2018080033-appb-000017
其中,Gk n表示第n次Gk(rssi)函数的输出值,即扫描范围值;rssi max为一个理论计算值,为一个常数;rssi n、rssi k分别表示第n次、第k次rssi的采集值;Kp为比例放大系数;Ki为积分放大系数;
Figure PCTCN2018080033-appb-000017
Where Gk n represents the output value of the nth Gk(rssi) function, ie the scan range value; rssi max is a theoretically calculated value, which is a constant; rssi n and rssi k represent the nth and kth rssi respectively Collected value; Kp is a proportional amplification factor; Ki is an integral amplification factor;
其中,通过卫星接收机的信号质量指示来确定是否对准卫星。Wherein, whether the satellite is aligned is determined by a signal quality indicator of the satellite receiver.
上述卫星跟踪方法,通过采集较少或者较低频率波束信号数据快速收敛卫星跟踪误差,通过不断的获取补偿角度来实时跟踪对准卫星,从而提高了卫星对准的精度和波束跟踪的精度,降低了时延和误差。同时能够很好适用于各种卫星波束追踪的需求。充分利用现有硬件条件资源,无需添加额外设备装置,进而降低了对伺服传动系统和姿态惯导系统精度的依赖。The above satellite tracking method quickly converges the satellite tracking error by collecting less or lower frequency beam signal data, and continuously tracks the alignment satellite by continuously obtaining the compensation angle, thereby improving the accuracy of satellite alignment and the accuracy of beam tracking, and reducing Delay and error. At the same time, it can be well adapted to the needs of various satellite beam tracking. Make full use of existing hardware condition resources without adding additional equipment, which reduces the dependence on the accuracy of servo drive system and attitude inertial navigation system.
附图说明DRAWINGS
图1为一实例中的卫星跟踪方法流程图;1 is a flow chart of a satellite tracking method in an example;
图2为一实施例中获取天线的方向性系数函数的流程图。2 is a flow chart of obtaining a directivity coefficient function of an antenna in an embodiment.
具体实施方式Detailed ways
为了使本发明的目的、技术方案及优点更加清楚明白,以下结合附图及实施例,对本发明进行进一步详细说明。应当理解,此处所描述的具体实施例仅仅用以解释本发明,并不用于限定本发明。The present invention will be further described in detail below with reference to the accompanying drawings and embodiments. It is understood that the specific embodiments described herein are merely illustrative of the invention and are not intended to limit the invention.
图1为一实施例的卫星跟踪方法流程图。该卫星跟踪方法用于实现卫星的快速跟踪对准,包括以下步骤S100~S500。1 is a flow chart of a satellite tracking method according to an embodiment. The satellite tracking method is used to implement fast tracking alignment of satellites, and includes the following steps S100-S500.
步骤S100,获取天线的方向性系数函数。In step S100, a directivity coefficient function of the antenna is obtained.
天线的方向性系数用以表示天线的集中辐射程度,具体的定义为:在总辐射功率相同的情况下,天线在最大辐射方向的辐射功率密度与均匀辐射在该方向的辐射功率密度的比值。天线的方向性系数其实就是天线的方向性系数函数。其中,首先根据不同天线类型进行理论上的计算,同时结合通过天线微波暗室测试获得的天线的方向图数据,将获取到的方向图数据按平均法合成一个方向图。对该方向图进行回归拟合生成一个的方向性系数函数。The directivity coefficient of the antenna is used to indicate the degree of concentrated radiation of the antenna, and is specifically defined as the ratio of the radiated power density of the antenna in the maximum radiation direction to the radiated power density of the uniform radiation in the direction in the case where the total radiated power is the same. The directivity coefficient of the antenna is actually the directivity coefficient function of the antenna. Firstly, according to different antenna types, the theoretical calculation is carried out, and the direction pattern data of the antenna obtained by the antenna microwave darkroom test is combined, and the obtained direction pattern data is synthesized into a pattern by the averaging method. A regression fit is applied to the pattern to generate a directivity coefficient function.
如图2所示,在一个实施例中,为天线的方向性系数函数的生成过程,包括:As shown in FIG. 2, in one embodiment, a process for generating a directivity coefficient function of an antenna includes:
步骤S110,采集天线不同频段的方向系数数据。Step S110, collecting direction coefficient data of different frequency bands of the antenna.
具体的,在一个实施例中,采集天线接收频段、发射频段的方向系数数据。Specifically, in an embodiment, the directional coefficient data of the antenna receiving frequency band and the transmitting frequency band are collected.
例如对于ka卫星天线,假定接收频段是18.7~19.2,发射频段是29.5~30.0。在接收频段内从中等间隔抽取10个频点。在发射频段内从中等间隔抽取10个频点。在天线微波暗室中分别采集这20个频点所对应的20组方向图数据。当然,这种采集方式是不限定的,还可以根据实际操作和需要对不同的卫星天线进行数据采集。For example, for the ka satellite antenna, it is assumed that the receiving frequency band is 18.7 to 19.2, and the transmitting frequency band is 29.5 to 30.0. 10 frequency points are extracted from the medium interval in the receive band. Extract 10 frequency points from the medium interval in the transmit band. The 20 sets of pattern data corresponding to the 20 frequency points are respectively collected in the antenna microwave darkroom. Of course, this collection method is not limited, and data acquisition can be performed on different satellite antennas according to actual operations and needs.
步骤S120,将所述不同频段的方向系数数据转换生成远场方向系数数据。Step S120, converting direction coefficient data of the different frequency bands to generate far-field direction coefficient data.
具体的,在一个实施例中,将采集到的天线接收频段的方向系数数据转换生成远场方向系数数据;将采集到的天线发射频段的方向系数数据转换生成远场方向系数数据。Specifically, in an embodiment, the collected direction coefficient data of the antenna receiving frequency band is converted to generate far-field direction coefficient data; and the direction coefficient data of the collected antenna transmitting frequency band is converted to generate far-field direction coefficient data.
步骤S130,根据所述远场方向系数数据选择与所述天线对应的拟合函数模型拟合生成方向性系数函数。Step S130, selecting a fitting function model corresponding to the antenna to generate a directivity coefficient function according to the far field direction coefficient data.
具体的,在一个实施例中,对于平面阵列天线,所述拟合函数模型为:Specifically, in one embodiment, for a planar array antenna, the fitting function model is:
Figure PCTCN2018080033-appb-000018
Figure PCTCN2018080033-appb-000018
其中J 1(x)为一阶贝塞尔函数,贝塞尔函数J α(x)是数学上的一类特殊函数的总称。贝塞尔函数为贝塞尔方程的解。通常单说的贝塞尔函数指第一类贝塞尔函数。贝塞尔函数的具体形式随贝塞尔方程中任意实数α变化而变化(相应地,α被称为其对应贝塞尔函数的阶数)。实际应用中最常见的情形为α是整数n,对应解称为n阶贝塞尔函数。J 1(x)为n为1时对应的贝塞尔方程的解。 Where J 1 (x) is a first-order Bessel function, and Bezier function J α (x) is a general term for a class of special functions in mathematics. The Bessel function is the solution of the Bessel equation. Usually the single-bessel function refers to the first type of Bessel function. The concrete form of the Bessel function varies with any real number α in the Bessel equation (correspondingly, α is called the order of its corresponding Bessel function). The most common case in practical applications is that α is an integer n and the corresponding solution is called an n-order Bessel function. J 1 (x) is the solution of the corresponding Bessel equation when n is 1.
在这里,贝塞尔函数中的
Figure PCTCN2018080033-appb-000019
u为一个一维阵列,包含两个角度值,一个H方向偏差角,一个V方向偏差角。
Here, in the Bessel function
Figure PCTCN2018080033-appb-000019
u is a one-dimensional array containing two angle values, one H-direction deviation angle, and one V-direction deviation angle.
其中,Az为通过天线微波暗室实际测量获取的天线的方位角差值;El为通过天线微波暗室实际测量获取的天线的俯仰角差值;h为常数,通过函数拟合时自动生成;Wherein, Az is the azimuth difference value of the antenna obtained by the actual measurement of the antenna microwave darkroom; El is the difference of the pitch angle of the antenna obtained by the actual measurement of the antenna microwave darkroom; h is a constant, which is automatically generated by function fitting;
将所述方位角差值Az和俯仰角差值El代入所述函数模型后得到方向性系数函数D(Az,El),D(Az,El)为一个两输入的函数。Substituting the azimuth difference value Az and the pitch angle difference value El into the function model yields a directivity coefficient function D(Az, El), and D(Az, El) is a two-input function.
对于反射面天线,所述拟合函数模型为:For a reflector antenna, the fit function model is:
Figure PCTCN2018080033-appb-000020
Figure PCTCN2018080033-appb-000020
其中J 1(x)为一阶贝塞尔函数,x=u;u=[Az El];u为一个一维阵列,包含两个角度值,一个H方向偏差角,一个V方向偏差角,这里可以理解为u=[Az El], Where J 1 (x) is a first-order Bessel function, x=u; u=[Az El]; u is a one-dimensional array containing two angular values, one H-direction deviation angle, and one V-direction deviation angle. This can be understood as u=[Az El],
Az为通过天线微波暗室实际测量获取的天线的方位角差值;El为通过天线微波暗室实际测量获取的天线的俯仰角差值;h为常数,通过函数拟合时自动生成;Az is the azimuth difference of the antenna obtained by the actual measurement of the antenna microwave darkroom; El is the difference of the pitch angle of the antenna obtained by the actual measurement of the antenna microwave darkroom; h is a constant, which is automatically generated by function fitting;
将所述天线的方位角差值Az和俯仰角差值El代入所述函数模型后得到方向性系数函数D(Az,El),D(Az,El)为一个两输入的函数。Substituting the azimuth difference Az and the pitch angle difference E of the antenna into the function model yields a directivity coefficient function D(Az, El), which is a two-input function.
步骤S200,获取所述方向性系数函数的雅可比矩阵,所述雅可比矩阵用于确定所述天线的角度补偿方向。Step S200: Acquire a Jacobian matrix of the directivity coefficient function, and the Jacobian matrix is used to determine an angle compensation direction of the antenna.
具体的,对获取到的方向性系数函数进行偏微分求导,得到雅可比矩阵,可以通过下列公式获得雅可比矩阵:Specifically, the obtained directional coefficient function is subjected to partial differential derivation to obtain a Jacobian matrix, and the Jacobian matrix can be obtained by the following formula:
所述
Figure PCTCN2018080033-appb-000021
Said
Figure PCTCN2018080033-appb-000021
其中,
Figure PCTCN2018080033-appb-000022
among them,
Figure PCTCN2018080033-appb-000022
其中,D(Az,El)为模拟生成的实际方向系数函数,D(Δθ n)为D(Az,El)的另一种表示形式,可以理解,D(Δθ n)=D(Az,El)。 Where D(Az, El) is the actual direction coefficient function generated by the simulation, and D(Δθ n ) is another representation of D(Az, El). It can be understood that D(Δθ n )=D(Az, El ).
步骤S300,通过扫描获取所述天线相对于卫星的偏差角矩阵,所述偏差角矩阵用于为获取补偿角度提供函数模型。Step S300, obtaining, by scanning, a matrix of deviation angles of the antenna with respect to a satellite, wherein the deviation angle matrix is used to provide a function model for acquiring a compensation angle.
具体的,在一个实施例中,通过扫描获取所述天线相对于卫星的偏差角矩阵,所述偏差角矩阵用于为获取补偿角度提供函数模型;通过扫描测量获取天线实际的方位角差值Az、俯仰角差值El;设所述
Figure PCTCN2018080033-appb-000023
则Δθ满足:
Specifically, in an embodiment, a matrix of deviation angles of the antenna relative to a satellite is obtained by scanning, the deviation angle matrix is used to provide a function model for acquiring a compensation angle; and the actual azimuth difference value Az of the antenna is obtained by scanning measurement , pitch angle difference E1;
Figure PCTCN2018080033-appb-000023
Then Δθ satisfies:
Figure PCTCN2018080033-appb-000024
Figure PCTCN2018080033-appb-000024
Figure PCTCN2018080033-appb-000025
Figure PCTCN2018080033-appb-000025
其中,Δθ和
Figure PCTCN2018080033-appb-000026
的算法是根据madgwick算法的推广应用,在这里
Figure PCTCN2018080033-appb-000027
为偏差角角速度矩阵,
Figure PCTCN2018080033-appb-000028
为Δθ对时间的求导;H=ωK,H为常数系数,ω为卫星的角速度;
Where Δθ and
Figure PCTCN2018080033-appb-000026
The algorithm is based on the promotion of the Madgwick algorithm, here
Figure PCTCN2018080033-appb-000027
For the angular angular velocity matrix,
Figure PCTCN2018080033-appb-000028
Is the derivative of Δθ versus time; H = ωK, H is a constant coefficient, and ω is the angular velocity of the satellite;
其中,Gk(rssi)为天线的扫描范围函数,大小由天线波束信号值rssi值决定;K Az为方位偏差角的扫描比例系数,K El为俯仰偏差角的扫描比例系数,扫描比例系数的大小根据天线的类型决定。 Where Gk(rssi) is the sweep range function of the antenna, the size is determined by the antenna beam signal value rssi value; K Az is the scan scale factor of the azimuth deviation angle, K El is the scan scale factor of the pitch deviation angle, and the scan scale factor is It is determined by the type of antenna.
在一个实施例中,扫描范围函数Gk(rssi)依据PI滤波器原理:In one embodiment, the scan range function Gk(rssi) is based on the PI filter principle:
Figure PCTCN2018080033-appb-000029
为一个常数;rssi n、rssi k分别表示第n次、第k次rssi的采集值;依据PI滤波器原理,Kp为比例放大系数;Ki为积分放大系数;
Figure PCTCN2018080033-appb-000029
It is a constant; rssi n and rssi k respectively represent the collected values of the nth and kth rssi; according to the principle of the PI filter, Kp is a proportional amplification factor; Ki is an integral amplification factor;
其中,通过自动变更扫描范围函数的扫描范围值Gk n的大小来进行螺旋渐进扫描。 Among them, the spiral progressive scan is performed by automatically changing the size of the scan range value Gk n of the scan range function.
步骤S400,根据所述方向性系数函数、所述偏差角矩阵、所述雅可比矩阵获取所述补偿角度,所述补偿角度用于指导所述天线在下一时刻进行移动。Step S400: Acquire the compensation angle according to the directivity coefficient function, the deviation angle matrix, and the Jacobian matrix, where the compensation angle is used to guide the antenna to move at a next moment.
根据所述方向性系数函数、所述偏差角矩阵、所述雅可比矩阵获取所述补偿角度,所述补偿角度用于指导所述天线在下一时刻进行移动。将获取到的方向性系数函数、偏差角矩阵、雅可比矩阵代入公式中获得补偿角度,进一步的,可以用以下的公式来获取补偿角度:Obtaining the compensation angle according to the directivity coefficient function, the deviation angle matrix, and the Jacobian matrix, and the compensation angle is used to guide the antenna to move at a next moment. The obtained directivity coefficient function, deviation angle matrix, and Jacobian matrix are substituted into the formula to obtain the compensation angle. Further, the following formula can be used to obtain the compensation angle:
补偿角度
Figure PCTCN2018080033-appb-000030
Compensation angle
Figure PCTCN2018080033-appb-000030
其中,among them,
Figure PCTCN2018080033-appb-000031
Figure PCTCN2018080033-appb-000031
Figure PCTCN2018080033-appb-000032
为计算的中间变量;Δθ n-1为n-1时刻的偏差角矩阵值;rssi n为第n次rssi的采集值;
Figure PCTCN2018080033-appb-000033
为雅可比矩阵;D(Az,El)为实际方向性系数函数;Δt为算法迭代周期;β为调节步长,对于不同类型的天线β的取值不同。
Figure PCTCN2018080033-appb-000032
For the calculated intermediate variable; Δθ n-1 is the deviation angle matrix value at time n-1; rssi n is the collected value of the nth rssi;
Figure PCTCN2018080033-appb-000033
It is a Jacobian matrix; D(Az, El) is the actual directivity coefficient function; Δt is the algorithm iteration period; β is the adjustment step size, and the values of different types of antennas β are different.
其中,当前时刻为n-1时刻,这里Δθ n-1的值是通过实际测量出来的,而根据Δθ n-1的值获得的Δθ n的值用于指导天线在下一时刻所要进行移动的角度。 Wherein, the current time is the time n-1, where the value of Δθ n-1 is actually measured, and the value of Δθ n obtained from the value of Δθ n-1 is used to guide the angle at which the antenna is to be moved at the next moment. .
步骤S500,在对准过程中动态获取所述补偿角度,并根据所述补偿角度不断调整所述天线扫描跟踪对准卫星。Step S500: dynamically acquiring the compensation angle during the alignment process, and continuously adjusting the antenna scan tracking alignment satellite according to the compensation angle.
具体的,在一个实施例中,在对准过程中动态获取所述补偿角度,并根据所述补偿角度不断调整所述天线扫描跟踪对准卫星。在对准的过程中,由于卫星实时在运动,所以需要根据卫星的运动来实时获取补偿角度,用以调整天线的方位角差值Az和俯仰角差值El来进一步的跟踪对准卫星。其中,对卫星的扫描方式采用螺旋渐进扫描,通过自动变更扫描范围函数的扫描范围值的大小来进行螺旋渐进扫描,Specifically, in one embodiment, the compensation angle is dynamically acquired during the alignment process, and the antenna scan tracking alignment satellite is continuously adjusted according to the compensation angle. In the process of alignment, since the satellite is moving in real time, it is necessary to obtain the compensation angle in real time according to the motion of the satellite, and to adjust the azimuth difference Az and the elevation angle difference E of the antenna to further track the satellite. Among them, the spiral scanning method is adopted for the scanning method of the satellite, and the spiral progressive scanning is performed by automatically changing the scanning range value of the scanning range function.
所述扫描范围函数Gk(rssi)依据PI滤波器原理:The scan range function Gk(rssi) is based on the principle of the PI filter:
Figure PCTCN2018080033-appb-000034
其中,Gk n表示第n次Gk(rssi)函数的输出值,即扫描范围值;rssi max为一个理论计算值,为一个常数;rssi n、rssi k分别表示第n次、第k次rssi的采集值;Kp为比例放大系数;Ki为积分放大系数;
Figure PCTCN2018080033-appb-000034
Where Gk n represents the output value of the nth Gk(rssi) function, ie the scan range value; rssi max is a theoretically calculated value, which is a constant; rssi n and rssi k represent the nth and kth rssi respectively Collected value; Kp is a proportional amplification factor; Ki is an integral amplification factor;
其中,通过卫星接收机的信号质量指示来确定是否对准卫星。具体的,当接收到的信号强度指示达到70%~80%时,说明天线已对准卫星的大致方位,当信号质量达40%左右,说明已对准卫星,也可以通过比如信号的eb/n0值大小来确定是否对准卫星。Wherein, whether the satellite is aligned is determined by a signal quality indicator of the satellite receiver. Specifically, when the received signal strength indication reaches 70% to 80%, it indicates that the antenna has been aligned with the general orientation of the satellite. When the signal quality is about 40%, it indicates that the satellite is aligned, and the signal may be eb/ The n0 value is used to determine if the satellite is aligned.
上述实施例,采取先大范围信号扫描使天线大致对上卫星波束,然后通过暗室模拟获取方向性系数函数,之后采用对方向性系数函数求解偏微分函数的方式来确定角度补偿方向和补偿角度,通过改变扫描范围值来实现螺旋渐进扫描,使得天线可以实现快速的跟踪对准卫星,同时提高了天线波束指向的精度;同时可以根据不同的动态特性自动调整天线的补偿角度,以自适应卫星;充分利用现有硬件资源,无需额外添加设备装置,也降低了跟踪精度对伺服系统和姿态惯导系统的依赖。In the above embodiment, the first large-scale signal scanning is performed to make the antenna substantially face the satellite beam, and then the directional coefficient function is obtained through the darkroom simulation, and then the directional coefficient function is used to solve the partial differential function to determine the angle compensation direction and the compensation angle. The spiral progressive scan is realized by changing the scan range value, so that the antenna can realize fast tracking and alignment to the satellite, and the accuracy of the antenna beam pointing is improved; and the compensation angle of the antenna can be automatically adjusted according to different dynamic characteristics to adapt the satellite; Making full use of existing hardware resources, without adding additional equipment, reduces the dependence of tracking accuracy on servo systems and attitude inertial navigation systems.
以上所述实施例仅表达了本发明的几种实施方式,其描述较为具体和详细,但并不能因此而理解为对本发明专利范围的限制。应当指出的是,对于本领域 的普通技术人员来说,在不脱离本发明构思的前提下,还可以做出若干变形和改进,这些都属于本发明的保护范围。因此,本发明专利的保护范围应以所附权利要求为准。The above-mentioned embodiments are merely illustrative of several embodiments of the present invention, and the description thereof is more specific and detailed, but is not to be construed as limiting the scope of the invention. It should be noted that a number of variations and modifications may be made by those skilled in the art without departing from the spirit and scope of the invention. Therefore, the scope of the invention should be determined by the appended claims.

Claims (9)

  1. 一种卫星跟踪方法,用于实现卫星的快速跟踪对准,其特征在于,包括:A satellite tracking method for realizing fast tracking alignment of satellites, characterized in that it comprises:
    获取天线的方向性系数函数;Obtaining a directivity coefficient function of the antenna;
    获取所述方向性系数函数的雅可比矩阵,所述雅可比矩阵用于确定所述天线的角度补偿方向;Obtaining a Jacobian matrix of the directivity coefficient function, wherein the Jacobian matrix is used to determine an angle compensation direction of the antenna;
    通过扫描获取所述天线相对于卫星的偏差角矩阵,所述偏差角矩阵用于为获取补偿角度提供函数模型;Obtaining, by scanning, a matrix of deviation angles of the antenna relative to a satellite, the deviation angle matrix being used to provide a function model for acquiring a compensation angle;
    根据所述方向性系数函数、所述偏差角矩阵、所述雅可比矩阵获取所述补偿角度,所述补偿角度用于指导所述天线在下一时刻进行移动;Obtaining the compensation angle according to the directivity coefficient function, the deviation angle matrix, and the Jacobian matrix, where the compensation angle is used to guide the antenna to move at a next moment;
    在对准过程中动态获取所述补偿角度,并根据所述补偿角度不断调整所述天线扫描跟踪对准卫星。The compensation angle is dynamically acquired during the alignment process, and the antenna scan tracking alignment satellite is continuously adjusted according to the compensation angle.
  2. 根据权利要求1所述的卫星跟踪方法,其特征在于,所述获取天线的方向性系数函数的步骤,包括:The satellite tracking method according to claim 1, wherein the step of acquiring a directivity coefficient function of the antenna comprises:
    采集天线不同频段的方向系数数据;Collecting direction coefficient data of different frequency bands of the antenna;
    将所述不同频段的方向系数数据转换生成远场方向系数数据;Converting the direction coefficient data of the different frequency bands to generate far-field direction coefficient data;
    根据所述远场方向系数数据选择与所述天线对应的拟合函数模型拟合生成方向性系数函数。A fitting function model fitting corresponding to the antenna is selected according to the far field direction coefficient data to generate a directivity coefficient function.
  3. 根据权利要求2所述的卫星跟踪方法,其特征在于,所述采集天线不同频段的方向系数数据的步骤,包括:The satellite tracking method according to claim 2, wherein the step of acquiring direction coefficient data of different frequency bands of the antenna comprises:
    采集天线接收频段、发射频段的方向系数数据。Collect the direction coefficient data of the antenna receiving band and the transmitting band.
  4. 根据权利要求2所述的卫星跟踪方法,其特征在于,The satellite tracking method according to claim 2, characterized in that
    对于平面阵列天线,所述拟合函数模型为:For a planar array antenna, the fit function model is:
    Figure PCTCN2018080033-appb-100001
    Figure PCTCN2018080033-appb-100001
    其中J 1(x)为一阶贝塞尔函数,
    Figure PCTCN2018080033-appb-100002
    u=[Az El],
    Where J 1 (x) is a first-order Bessel function,
    Figure PCTCN2018080033-appb-100002
    u=[Az El],
    Az为通过天线微波暗室实际测量获取的天线的方位角差值;El为通过天线微波暗室实际测量获取的天线的俯仰角差值;h为常数,通过函数拟合时自动生 成;Az is the azimuth difference of the antenna obtained by the actual measurement of the antenna microwave darkroom; El is the difference of the pitch angle of the antenna obtained by the actual measurement of the antenna microwave darkroom; h is a constant, which is automatically generated by function fitting;
    将所述方位角差值Az和俯仰角差值El代入所述函数模型后得到方向性系数函数D(Az,El);Substituting the azimuth difference value Az and the pitch angle difference value El into the function model to obtain a directivity coefficient function D(Az, El);
    对于反射面天线,所述拟合函数模型为:For a reflector antenna, the fit function model is:
    Figure PCTCN2018080033-appb-100003
    Figure PCTCN2018080033-appb-100003
    其中J 1(x)为一阶贝塞尔函数,x=u;u=[Az El]; Where J 1 (x) is a first-order Bessel function, x=u; u=[Az El];
    Az为通过天线微波暗室实际测量获取的天线的方位角差值;El为通过天线微波暗室实际测量获取的天线的俯仰角差值;h为常数,通过函数拟合时自动生成;Az is the azimuth difference of the antenna obtained by the actual measurement of the antenna microwave darkroom; El is the difference of the pitch angle of the antenna obtained by the actual measurement of the antenna microwave darkroom; h is a constant, which is automatically generated by function fitting;
    将所述天线的方位角差值Az和俯仰角差值El代入所述函数模型后得到方向性系数函数D(Az,El)。Substituting the azimuth difference value Az and the pitch angle difference value E of the antenna into the function model yields a directivity coefficient function D(Az, El).
  5. 根据权利要求1所述的卫星跟踪方法,其特征在于,所述获取所述方向性系数函数的雅可比矩阵,所述雅可比矩阵用于确定所述天线的角度补偿方向的步骤,包括:The satellite tracking method according to claim 1, wherein the step of acquiring a Jacobian matrix of the directivity coefficient function, wherein the Jacobian matrix is used to determine an angle compensation direction of the antenna comprises:
    所述
    Figure PCTCN2018080033-appb-100004
    Said
    Figure PCTCN2018080033-appb-100004
    其中,
    Figure PCTCN2018080033-appb-100005
    among them,
    Figure PCTCN2018080033-appb-100005
    其中,D(Δθ n)为D(Az,El)的另一种表示形式。 Where D(Δθ n ) is another representation of D(Az, El).
  6. 根据权利要求1所述的卫星跟踪方法,其特征在于,所述通过扫描获取所述天线相对于卫星的偏差角矩阵,所述偏差角矩阵用于为获取补偿角度提供函数模型的步骤,包括:The satellite tracking method according to claim 1, wherein the step of acquiring a deviation angle matrix of the antenna with respect to a satellite by scanning, the deviation angle matrix is used for providing a function model for acquiring a compensation angle, comprising:
    通过扫描测量获取天线实际的方位角差值Az、俯仰角差值El,设所述偏差角矩阵
    Figure PCTCN2018080033-appb-100006
    则Δθ满足:
    Obtaining the actual azimuth difference value Az and the pitch angle difference value El of the antenna by scanning measurement, and setting the deviation angle matrix
    Figure PCTCN2018080033-appb-100006
    Then Δθ satisfies:
    Figure PCTCN2018080033-appb-100007
    Figure PCTCN2018080033-appb-100007
    Figure PCTCN2018080033-appb-100008
    Figure PCTCN2018080033-appb-100008
    其中,
    Figure PCTCN2018080033-appb-100009
    为偏差角角速度矩阵,
    Figure PCTCN2018080033-appb-100010
    为Δθ对时间的求导;H=ωK,H为常数系数;其中Gk(rssi)为扫描范围函数,大小由天线波束信号值rssi值决定;K Az、K El为扫描比例系数。
    among them,
    Figure PCTCN2018080033-appb-100009
    For the angular angular velocity matrix,
    Figure PCTCN2018080033-appb-100010
    It is the derivative of Δθ versus time; H=ωK, H is a constant coefficient; where Gk(rssi) is a function of the scan range, and the size is determined by the value of the antenna beam signal value rssi; K Az and K El are the scan scale coefficients.
  7. 根据权利要求6所述的卫星跟踪方法,其特征在于,所述扫描范围函数Gk(rssi)依据PI滤波器原理:The satellite tracking method according to claim 6, wherein the scan range function Gk(rssi) is based on a PI filter principle:
    Figure PCTCN2018080033-appb-100011
    为一个常数;rssi n、rssi k分别表示第n次、第k次rssi的采集值;Kp为比例放大系数;Ki为积分放大系数;
    Figure PCTCN2018080033-appb-100011
    Is a constant; rssi n and rssi k respectively represent the collected values of the nth and kth rssi; Kp is a proportional amplification factor; Ki is an integral amplification factor;
    其中,通过自动变更扫描范围函数的扫描范围值的大小来进行螺旋渐进扫描。Among them, the spiral progressive scan is performed by automatically changing the size of the scan range value of the scan range function.
  8. 根据权利要求1所述的卫星跟踪方法,其特征在于,所述根据所述方向性系数函数、所述偏差角矩阵、所述雅可比矩阵获取所述补偿角度,所述补偿角度用于指导所述天线在下一时刻进行移动的步骤,包括:The satellite tracking method according to claim 1, wherein the compensation angle is obtained according to the directivity coefficient function, the deviation angle matrix, and the Jacobian matrix, and the compensation angle is used for guiding a location The step of moving the antenna at the next moment includes:
    所述补偿角度
    Figure PCTCN2018080033-appb-100012
    The compensation angle
    Figure PCTCN2018080033-appb-100012
    其中,among them,
    Figure PCTCN2018080033-appb-100013
    Figure PCTCN2018080033-appb-100013
    Figure PCTCN2018080033-appb-100014
    为计算的中间变量;Δθ n-1为n-1时刻的偏差角矩阵值;rssi n为第n次rssi的采集值;
    Figure PCTCN2018080033-appb-100015
    为雅可比矩阵;D(Az,El)为实际方向性系数函数;Δt为算法迭代周期;β为调节步长,对于不同类型的天线β的取值不同。
    Figure PCTCN2018080033-appb-100014
    For the calculated intermediate variable; Δθ n-1 is the deviation angle matrix value at time n-1; rssi n is the collected value of the nth rssi;
    Figure PCTCN2018080033-appb-100015
    It is a Jacobian matrix; D(Az, El) is the actual directivity coefficient function; Δt is the algorithm iteration period; β is the adjustment step size, and the values of different types of antennas β are different.
  9. 根据权利要求1所述的卫星跟踪方法,其特征在于,所述在对准过程中动态获取所述补偿角度,并根据所述补偿角度不断调整所述天线扫描跟踪对准卫星的步骤,包括:The satellite tracking method according to claim 1, wherein the step of dynamically acquiring the compensation angle during the alignment process and continuously adjusting the antenna scan tracking alignment satellite according to the compensation angle comprises:
    根据所述补偿角度不断调整所述天线的方位角差值Az和俯仰角差值El螺旋渐进扫描跟踪对准卫星;And continuously adjusting the azimuth difference value Az and the pitch angle difference value of the antenna according to the compensation angle; the spiral progressive scan tracking alignment satellite;
    其中,通过自动变更扫描范围函数的扫描范围值的大小来进行螺旋渐进扫描,Wherein, the spiral progressive scan is performed by automatically changing the size of the scan range value of the scan range function,
    所述扫描范围函数Gk(rssi)依据PI滤波器原理:The scan range function Gk(rssi) is based on the principle of the PI filter:
    Figure PCTCN2018080033-appb-100016
    其中,Gk n表示第n次Gk(rssi)函数的输出值,即扫描范围值;rssi max为一个理论计算值,为一个常数;rssi n、rssi k分别表示第n次、第k次rssi的采集值;Kp为比例放大系数;Ki为积分放大系数;
    Figure PCTCN2018080033-appb-100016
    Where Gk n represents the output value of the nth Gk(rssi) function, ie the scan range value; rssi max is a theoretically calculated value, which is a constant; rssi n and rssi k represent the nth and kth rssi respectively Collected value; Kp is a proportional amplification factor; Ki is an integral amplification factor;
    其中,通过卫星接收机的信号质量指示来确定是否对准卫星。Wherein, whether the satellite is aligned is determined by a signal quality indicator of the satellite receiver.
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